Weyl conformal symmetry model of the dark galactic halo
R. K. Nesbet

TL;DR
This paper proposes a Weyl conformal symmetry-based model that explains galactic halo dynamics and cosmic acceleration without dark matter, fitting observations with minimal parameters.
Contribution
It introduces a conformal Higgs model that accounts for galactic rotation curves and cosmic acceleration without dark matter, using Weyl symmetry modifications.
Findings
Fits observed galactic rotation velocities without dark matter
Accurately models cosmic acceleration with one free parameter
Provides a unified conformal framework for gravity and Higgs field
Abstract
The postulate of universal conformal (local Weyl scaling) symmetry modifies both general relativity and the Higgs scalar field model. The conformal Higgs model (CHM) generates an effective cosmological constant that fits observed accelerating Hubble expansion for redshifts (7.33 Gyr) accurately with only one free parameter. Growth of a galaxy is modeled by central accumulation of matter from an enclosing empty spherical halo whose radius expands with depletion. Details of this process account for the nonclassical radial centripetal acceleration observed as excessive orbital velocities in galactic haloes. There is no need for dark matter.
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Taxonomy
TopicsCosmology and Gravitation Theories · Astronomy and Astrophysical Research · Scientific Research and Discoveries
